activity
20132026
most citedIMAGINE: A comprehensive view of the interstellar medium, Galactic magnetic fields and cosmic rays

77 citations · 710 across the 58 of their papers we have counts for

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Showing 2026Show all

11 papers · 1 filter

astro-ph.GA2026

The impact of the turbulent Mach number on star formation and the initial mass function

Sajay Sunny Mathew, Christoph Federrath, Amit Seta

Turbulence regulates star formation by influencing the density structure and fragmentation of molecular clouds, and therefore it is expected to play a key role in setting the initi…

astro-ph.GA2026

Cosmic-ray electron propagation in the peculiar barred spiral galaxy NGC 2442

Shengtao Wang, Xiaohui Sun, Volker Heesen +13

Face-on spiral galaxies offer a favorable geometry for studying magnetic-field structures and cosmic-ray (CR) propagation because projection effects and structural overlap are redu…

astro-ph.CO2026

Probing the Baryon Distribution with Fast Radio Bursts

Manisha Caleb, Jéferson A. S. Fortunato, Steffen Hagstotz +12

Baryonic feedback redistributes matter on small to mid cosmological scales, ultimately limiting inferences from Stage IV galaxy surveys. Direct baryon tracers are crucial for recov…

astro-ph.HE2026

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM

Kohei Kurahara, Takuya Akahori, Amit Seta +5

This chapter proposes a research framework to quantitatively investigate non-thermal components in the Intracluster Medium (ICM) of galaxy clusters, which are critical ingredients…

astro-ph.GA2026

Probing Magnetic Fields In and Around Galaxies Near and Far

S. A. Mao, Rainer Beck, Aritra Basu +14

In order to understand the magnetization of galaxies and the role of magnetic fields in feedback processes that govern star formation and galaxy evolution, it is essential to have…

astro-ph.CO2026

Fast Radio Bursts as Cosmological Probes

Manisha Caleb, Jéferson A. S. Fortunato, Steffen Hagstotz +14

Fast radio bursts (FRBs) are brief, coherent radio pulses of extragalactic origin. They typically last from microseconds to milliseconds and have energies large enough to be visibl…